Wide-field Low-z SN Search with the NOAO Mosaic

Details Wide-field Low-z SN Search with the NOAO Mosaic Wide-field Low-z SN Search with the NOAO Mosaic

Aug 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000noao.prop..422s&link_type=abstract

NOAO Proposal ID #2000B-0422

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While observations of distant supernovae (SNe) are providing intriguing new information about cosmological parameters, there is still much work to be done on understanding the details of the various types of SNe and the possible systematic uncertainties in their use as precise distance indicators. Such work is best done with studies of relatively nearby SNe (z ≤ 0.1), which are bright enough to obtain detailed photometric and spectroscopic follow-up. We propose to conclude our successful Nearby Galaxies Supernova Search (NGSS) conducting a wide- field CCD search for nearby SNe using the KPNO 0.9m telescope with the NOAO Mosaic. Continuing detailed observations of these nearby SNe, made possible by the coordination of SN programs worldwide, will allow us to determine accurate SN rates by SN subclass, and study the variety of "peculiar" type I and II events SNe which continue to elude our understanding due to the low numbers of known examples and limited organized follow-up observations.

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